A dataset provided by the European Space Agency

Name: Two LMC Superbubbles With Evidence of SNR Shocks
Published: 2009-04-11T00:00:00Z

Proposal ID	050368
Title	Two LMC Superbubbles With Evidence of SNR Shocks
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0503680101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0503680201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0503680401
DOI	https://doi.org/10.5270/esa-3dgketc
Principal Investigator, PI	Dr Rosa Williams
Abstract	Superbubbles (SBs) are formed by the combined actions of stellar winds andsupernova explosions from massive stars in OB associations. These objectscontribute significantly to the hot gas component of a galaxy.s interstellarmedium (ISM), as well as affecting the structure of the ISM to large scales. Wepropose XMM-Newton observations of two SBs in the Large Magellanic Cloud, N70and N185, with indicators of recent interior SNe. From their X-ray spectra, wewill investigate (a) enhanced abundances indicating recent enrichment by SNejecta; (b) the energy budgets of the SBs, and whether those are consistent withexpected stellar-wind inputs; and (c) the required input of SNRs to these SBs toobtain the observed energies.
Publications	Quasi-stellar Object Selection Algorithm Using Time Variability and Machine Learning: Selection of 1620 Quasi-stellar Object Candidates from MACHO Large Magellanic Cloud Database \|Kim, Dae-Won, Protopapas, Pavlos, et al. \| ApJ \| 735-68 \| 2011 \| 2011ApJ...735...68K \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...735...68K A Refined QSO Selection Method Using Diagnostics Tests: 663 QSO Candidates in the Large Magellanic Cloud \|Kim, Dae-Won, Protopapas, Pavlos, et al. \| ApJ \| 747-107 \| 2012 \| 2012ApJ...747..107K \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...747..107K The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens, Nicola, Romer, A. Kathy, et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies, E. J., Romer, A. Kathy, et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter, J. A., Semba, S., \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C Multi-frequency Observations of a Superbubble in the LMC: The Case of LHA 120-N 70 \|De Horta, A. Y., Sommer, E. R., et al. \| AJ \| 147-162 \| 2014 \| 2014AJ....147..162D \| http://ui.adsabs.harvard.edu/#abs/2014AJ....147..162D Physical Nature of the S II-bright Shell Nebulae N70 and N185 \|Zhang, Ning-Xiao, Chu, You-Hua, et al. \| ApJ \| 792-58 \| 2014 \| 2014ApJ...792...58Z \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...792...58Z RBS 1032: A Tidal Disruption Event in Another Dwarf Galaxy? \|Maksym, W. Peter, Lin, Dacheng, \| ApJ \| 792-29 \| 2014 \| 2014ApJ...792L..29M \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...792L..29M Diffuse X-Ray Emission from the Superbubbles N70 and N185 in the Large Magellanic Cloud \|Reyes-Iturbide, J., Rosado, M., et al. \| AJ \| 148-102 \| 2014 \| 2014AJ....148..102R \| http://ui.adsabs.harvard.edu/#abs/2014AJ....148..102R Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov, V. N., \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao, Weike, Chen, Chen, et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X The population of X-ray supernova remnants in the Large Magellanic Cloud \|Maggi, P., Haberl, F., et al. \| A&A \| 585-162 \| 2016 \| 2016A&A...585A.162M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...585A.162M The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Identification of high-mass X-ray binaries selected from XMM-Newton observations of the LMC* \|van Jaarsveld, N., Buckley, D. A. H., et al. \| MNRAS \| 475-3253 \| 2018 \| 2018MNRAS.475.3253V \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.3253V Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas, Konstantinos, Reiprich, Thomas H., \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The XMM Cluster Survey: Present status and latest results \|Viana, P. T. P., Mehrtens, N., et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC \|Ou, Po-Sheng, Chu, You-Hua, et al. \| ApJ \| 863-137 \| 2018 \| 2018ApJ...863..137O \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...863..137O Testing emergent gravity on galaxy cluster scales \|Tamosiunas, Andrius, Bacon, David, et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood, Devon L., Jeltema, Tesla, et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese, A., Annis, J., et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P New optically identified supernova remnants in the Large Magellanic Cloud \|Yew, Miranda, Filipovi\\u0107, Miroslav D., et al. \| MNRAS \| 500-2336 \| 2021 \| 2021MNRAS.500.2336Y \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500.2336Y Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2008-01-26T16:11:46Z/2008-03-11T03:31:39Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2009-04-11T00:00:00Z
Keywords	"magellanic cloud", "supernova remnant", "energy budgets", "XMM-Newton", "lmc superbubbles", "supernova remnant shoc", "ob associations", "xmm newton", "superbubbles sbs", "interstellar medium ism", "stellar wind inputs", "xray spectra", "XMM", "supernova explosions", "massive stars", "combined actions", "interior sne", "hot gas component", "enrichment bysupernovaejecta", "stellar winds", "enhanced abundance"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Rosa Williams, 2009, 'Two LMC Superbubbles With Evidence of SNR Shocks', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-3dgketc